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@ARTICLE{Jia:185611,
      author       = {Jia, J. Y. and Preusse, P. and Ern, M. and Chun, H.-Y. and
                      Gille, J. C. and Eckermann, S. D. and Riese, M.},
      title        = {{S}ea surface temperature as a proxy for convective gravity
                      wave excitation: a study based on global gravity wave
                      observations in the middle atmosphere},
      journal      = {Annales geophysicae},
      volume       = {32},
      number       = {11},
      issn         = {1432-0576},
      address      = {Katlenburg, Lindau},
      publisher    = {Copernicus},
      reportid     = {FZJ-2014-07037},
      pages        = {1373 - 1394},
      year         = {2014},
      abstract     = {Absolute values of gravity wave momentum flux (GWMF)
                      deduced from satellite measurements by the Sounding of the
                      Atmosphere using Broadband Emission Radiometry (SABER)
                      instrument and the High Resolution Dynamics Limb Sounder
                      (HIRDLS) are correlated with sea surface temperature (SST)
                      with the aim of identifying those oceanic regions for which
                      convection is a major source of gravity waves (GWs). Our
                      study identifies those latitude bands where high correlation
                      coefficients indicate convective excitation with confidence.
                      This is based on a global ray-tracing simulation, which is
                      used to delineate the source and wind-filtering effects.
                      Convective GWs are identified at the eastern coasts of the
                      continents and over the warm water regions formed by the
                      warm ocean currents, in particular the Gulf Stream and the
                      Kuroshio. Potential contributions of tropical cyclones to
                      the excitation of the GWs are discussed. Convective
                      excitation can be identified well into the mid-mesosphere.
                      In propagating upward, the centers of GWMF formed by
                      convection shift poleward. Some indications of the main
                      forcing regions are even shown for the upper
                      mesosphere/lower thermosphere (MLT).},
      cin          = {IEK-7},
      ddc          = {550},
      cid          = {I:(DE-Juel1)IEK-7-20101013},
      pnm          = {234 - Composition and Dynamics of the Upper Troposphere and
                      Stratosphere (POF2-234)},
      pid          = {G:(DE-HGF)POF2-234},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000345785000001},
      doi          = {10.5194/angeo-32-1373-2014},
      url          = {https://juser.fz-juelich.de/record/185611},
}